1868 Thersites

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1868 Thersites
Discovery [1]
Discovered byC. J. van Houten
I. van Houten G.
T. Gehrels
Discovery sitePalomar Obs.
Discovery date24 September 1960
Designations
(1868) Thersites
Pronunciation/θərˈsaɪtiːz/[7]
Named after
Thersites [2]
(Greek mythology)
2008 P-L · 1972 RB2
Minor planet category
Jupiter trojan [1][3][4]
Greek [5][6] · background [6]
Orbital characteristics [3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc63.50 yr (23,195 d)
Aphelion5.9015 AU
Perihelion4.7316 AU
5.3166 AU
Eccentricity0.1100
12.26 yr (4,478 d)
277.51°
0° 4m 49.44s / day
Inclination16.751°
197.82°
169.76°
Jupiter MOID0.2116 AU
TJupiter2.9030
Physical characteristics
Mean diameter
68.16±0.81 km[8]
70.08 km (calculated)[4]
78.89±2.02 km[9]
10.412±0.003 h[a]
10.416±0.014 h[10]
10.48±0.01 h[11][b]
0.055±0.003[9]
0.055±0.008[8]
0.057 (assumed)[4]
C (assumed)[4]
V–I = 0.960±0.034[4]
Absolute magnitude (H)
9.30[9]
9.5[1][3][4]
9.6[8]

1868 Thersites /θərˈsaɪtiːz/ is a large Jupiter trojan from the Greek camp, approximately 70 kilometers (43 miles) in diameter. Discovered during the Palomar–Leiden survey at Palomar in 1960, it was later named after the warrior Thersites from Greek mythology. The presumed carbonaceous C-type asteroid belongs to the 50 largest Jupiter trojans and has a rotation period of 10.48 hours.[4]

Discovery[]

Thersites was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Tom Gehrels at the Palomar Observatory in California.[1] On the same day, the group discovered another Jupiter trojan, 1869 Philoctetes.

The body's observation arc begins with a precovery taken at Palomar in March 1954, more than 6 years prior to its official discovery observation.[1]

Palomar–Leiden survey[]

The provisional survey designation "P-L" stands for Palomar–Leiden, named after the Palomar and Leiden observatories, which collaborated on the fruitful Palomar–Leiden survey in the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope, also known as the 48-inch Schmidt Telescope, and shipped the photographic plates to Cornelis and Ingrid van Houten at Leiden Observatory, where astrometry was carried out. The trio are credited with the discovery of several thousand minor planets.[12]

Orbit and classification[]

Thersites is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's L4 Lagrangian point, 60° ahead of the Gas Giant's orbit in a 1:1 resonance (see Trojans in astronomy). It is also a non-family asteroid in the Jovian background population.[6][13] It orbits the Sun at a distance of 4.7–5.9 AU once every 12 years and 3 months (4,478 days; semi-major axis of 5.32 AU). Its orbit has an eccentricity of 0.11 and an inclination of 17° with respect to the ecliptic.[3]

Physical characteristics[]

The Trojan asteroid has been assumed to be a carbonaceous C-type asteroid.[4]

Rotation period[]

In July 1994, a first rotational lightcurve of Thersites was obtained from photometric observations by Italian astronomer Stefano Mottola using the former Dutch 0.9-metre Telescope at ESO's La Silla Observatory in northern Chile. Lightcurve analysis gave a rotation period of 10.416±0.014 hours with a brightness variation of 0.14±0.01 magnitude (U=2+).[4][10] The best-rated lightcurve by Robert Stephens at the Center for Solar System Studies from June 2016 gave a period of 10.48 hours and an amplitude of 0.27 magnitude (U=3-).[4][11][b] Follow-up observation in 2017 gave a similar period of 10.412 hours (U=2).[a]

Diameter and albedo[]

According to the space-based surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Thersites has a low albedo of 0.055 and measures 78.9 and 68.2 kilometers in diameter, respectively.[8][9] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057, and calculates an intermediate diameter of 70.08 kilometers with an absolute magnitude of 9.5.[4]

100+ largest Jupiter trojans

Naming[]

This minor planet was named from Greek mythology after Thersites, a Greek warrior who wanted to abandon Troy's siege during the Trojan War and head home. The given name also refers to the fact, that the asteroid was discovered farthest from the L4 Lagrangian point.[2] The official naming citation was published by the Minor Planet Center on 1 June 1975 (M.P.C. 3826).[14]

Notes[]

  1. ^ Jump up to: a b Stephens (2017). Observations from July 2017. (lightcurve plot) Rotation period 10.412±0.003 hours with a brightness amplitude of 0.18±0.01 mag. Quality code of 2. Summary figures for (1868) Thersites at the LCDB.
  2. ^ Jump up to: a b Lightcurve plot of (1868) Thersites (July 2016) Rotation period 10.48±0.01 hours with a brightness amplitude of 0.27±0.02 mag. Quality code is 3-. Summary figures for at the LCDB.

References[]

  1. ^ Jump up to: a b c d e "1868 Thersites (2008 P-L)". Minor Planet Center. Retrieved 9 June 2018.
  2. ^ Jump up to: a b Schmadel, Lutz D. (2007). "(1868) Thersites". Dictionary of Minor Planet Names – (1868) Thersites. Springer Berlin Heidelberg. p. 150. doi:10.1007/978-3-540-29925-7_1869. ISBN 978-3-540-00238-3.
  3. ^ Jump up to: a b c d "JPL Small-Body Database Browser: 1868 Thersites (2008 P-L)" (2017-09-28 last obs.). Jet Propulsion Laboratory. Retrieved 9 June 2018.
  4. ^ Jump up to: a b c d e f g h i j k "LCDB Data for (1868) Thersites". Asteroid Lightcurve Database (LCDB). Retrieved 9 June 2018.
  5. ^ "List of Jupiter Trojans". Minor Planet Center. 31 May 2018. Retrieved 9 June 2018.
  6. ^ Jump up to: a b c "Asteroid (1868) Thersites". AstDyS-2, Asteroids – Dynamic Site. Retrieved 20 October 2019.
  7. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  8. ^ Jump up to: a b c d Grav, T.; Mainzer, A. K.; Bauer, J. M.; Masiero, J. R.; Nugent, C. R. (November 2012). "WISE/NEOWISE Observations of the Jovian Trojan Population: Taxonomy". The Astrophysical Journal. 759 (1): 10. arXiv:1209.1549. Bibcode:2012ApJ...759...49G. doi:10.1088/0004-637X/759/1/49. S2CID 119101711. (online catalog)
  9. ^ Jump up to: a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
  10. ^ Jump up to: a b Mottola, Stefano; Di Martino, Mario; Erikson, Anders; Gonano-Beurer, Maria; Carbognani, Albino; Carsenty, Uri; et al. (May 2011). "Rotational Properties of Jupiter Trojans. I. Light Curves of 80 Objects". The Astronomical Journal. 141 (5): 32. Bibcode:2011AJ....141..170M. doi:10.1088/0004-6256/141/5/170.
  11. ^ Jump up to: a b Stephens, Robert D.; Coley, Daniel R.; Warner, Brian D.; French, Linda, M. (October 2016). "Lightcurves of Jovian Trojan Asteroids from the Center for Solar System Studies: L4 Greek Camp and Spies". The Minor Planet Bulletin. 43 (4): 323–331. Bibcode:2016MPBu...43..323S. ISSN 1052-8091. Retrieved 9 June 2018.
  12. ^ "Minor Planet Discoverers". Minor Planet Center. 31 May 2018. Retrieved 9 June 2018.
  13. ^ "Asteroid 1868 Thersites". Small Bodies Data Ferret. Retrieved 9 June 2018.
  14. ^ Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221. Bibcode:2009dmpn.book.....S. doi:10.1007/978-3-642-01965-4. ISBN 978-3-642-01964-7.

External links[]

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